Name
deep2iraf
Purpose
The
deep2iraf.cl task provides a
quick-and-dirty way to convert spectra generated by the
DEEP2 DEIMOS data reduction pipeline
into a format readable by IRAF.
Type
IRAF CL script
Author
Gregory D. Wirth,
W. M. Keck Observatory
Installation
- install this file in your home iraf directory
- execute (or add to your loginuser.cl file) this line:
task deep2iraf = home$deep2iraf.cl
Examples
- Convert DEEP2 spectrum into IRAF-compatible image koo.fits:
deep2iraf spec1d.KTRS02.031.1833.fits out=koo.fits
- Run "mysplot" on the DEEP2 spectrum without leaving a new
file behind:
deep2iraf spec1d.KTRS02.031.1833.fits domysplot+
Restrictions
Must be run from a directory in which the user has access to
generate temporary files.
Side Effects
The resulting spectrum is linearized and hence rebinned. CAVEAT
EMPTOR!!!
Go to:
DEIMOS Home Page -
Instruments Home Page -
Keck Home Page
Last modified: Mon Dec 22 21:58:11 HST 2008